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Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere

  • Authors: Juan Martínez-Sykora, Bart De Pontieu, Mats Carlsson, Viggo H. Hansteen, Daniel Nóbrega-Siverio, and Boris V. Gudiksen

2017 The Astrophysical Journal 847 36.

  • Provider: AAS Journals

Caption: Figure 6.

Temperature, in logarithmic scale, for the GOL simulation at t = 1260 s (top left), 1350 s (bottom left), 1445 s (top right), and 1540 s (bottom right) with magnetic field lines shown in white. In the beginning (left panels) the thermodynamic structures are aligned with the magnetic field, whereas at later times (right panels) the magnetic connectivity has changed and the alignment is poor (see corresponding Movie 1).

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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